Concept Review CH. 15 Flashcards
Suppose f is a continuous function defined on a rectangle R = [a,b] x [c,d]. Write an expression for double Riemann Sum of f. If f(x,y) >= 0, what does sum represent?
How is Midpoint Rule Used?
ΣΣ (f (xij, yij) Delta A.
If it is greater than 0 then it represents the volume underneath the rectangle.
Midpoint Rule just means f(xij, yij) is the centers of these rectangles.
Definition of ∫∫ f(x,y) dA over R as a limit?
Lim n,m -> ∞ ΣΣ (f xij, yij) Delta A
What is the Geometric Interpretation of ∫∫ f(x,y) dA over R if f(x,y) >= 0? What if f takes on both positive and negative values?
If f(x,y) >= 0, the integral represents the volume of the solid that lies above the rectangle R and below the surface z = f(x,y). If f takes on positive and negative values, then ∫∫ f(x,y) dA = V1 - V2. Where V1 is volume above R and below z = f(x,y). V2 is volume below R and above the surface.
What is Fubini’s Theorem?
∫∫ f(x,y) dA = ∫a,b∫ c,d f(x,y) dxdy =
∫c,d∫ a,b f(x,y) dydx.
How do you find the average value of f?
avg(f) = 1/A(R) ∫∫ f(x,y) dA . A(R) = area of R, so if triangle, then find area of triangle you are iterating over.
How do you define ∫∫D f(x,y) dA if D is a bounded region that is not a rectangle? What about for Triple Integrals?
Since D is bounded, then it can be enclosed in a rectangular region R. We define a new function F with domain R as F(x,y) = { f(x,y) if (x,y) is in D 0 if (x,y) is in R, but not in D. } Then ∫∫D f(x,y) dA = ∫∫R F(x,y) dA
Same process for triple integrals.
What is the difference between a type 1 region and a type 2 region in R^2?
Type 1 means that the region D of ∫∫D f(x,y) dA lies between the graphs of two continuous functions of x, that is D = {x,y | a <= x <= b, g1(x) <= y <= g2(x)}.
Type 2 means it lies between the graphs of two functions of y, thus
D = {(x,y) | a <= y <= b, g1(y) <= x <= g2(y)}.
What are the properties of Double Integrals?
They follow the same properties as Integrals. You know this and you can easily do double integrals.
How do you change from rectangular coordinates to polar coordinates and why would you want to?
If we can more easily describe the region D in polar coordinates then we should make the change to polar coordinates.
D = { (r, θ) | a <= θ <= b, h1(θ) <= r <= h2(θ) }
x = r *cos(θ)
y = r *sin(θ)
dA = rdrdθ
If a Plane region D has a density function p(x,y), then how do we find the mass, moments about the axes, and the center of mass?
mass = ∫∫D p(x,y) dA
Moments:
Mx = ∫∫D yp(x,y) dA
My = ∫∫D xp(x,y) dA
Center of Mass:
X = My/m
Y = Mx/m
(My/m, Mx/m)
What is the equation for finding the surface area from a given function?
A(S) = ∫∫D √( (dx)^2 + (dy)^2 + 1 ) dA assuming dx and dy are the derivatives with respect to x and respect to y and assuming that they are continuous.
What is the definition of a triple integral over a rectangular box B?
∫∫∫B f (x, y, z)dV = lim l,m, n -> ∞ ΣΣΣ f(xij, yij, zij) V.
V is the volume of each sub box.
Evaluate the same way as with double integrals.
What is the difference between a Type 1 Region and Type 2 Region and Type 3 Region in R^3?
Type 1 if it lies between the graphs of two continuous functions of x and y, that is,
E = { (x,y,z)| (x,y) in D, u1(x,y) <= z <= u2(x,y) }
∫∫∫B f (x, y, z)dV = ∫∫ [ ∫u2(x,y) u1(x,y) f (x, y, z)dz ]dA
Type 2 if it lies between the graphs of two continuous functions of z and y, that is,
E = { (x,y,z)| (y, z) in D, u1(y, z) <= x <= u2(y,z) }
∫∫∫B f (x, y, z)dV = ∫∫ [ ∫u2(y, z) u1(y,z) f (x, y, z)dx ]dA
Type 3 if it lies between the graphs of two continuous functions of x and z, that is,
E = { (x,y,z)| (x,z) in D, u1(x,z) <= y <= u2(x,z) }
∫∫∫B f (x, y, z)dV = ∫∫ [ ∫u2(x,z) u1(x,z) f (x, y, z)dy ]dA
What are the Mass, Center of Mass, Moments, and Center of Mass for Triple Integrals
m = ∫∫∫E p(x, y, z)dV for density function p.
Moments:
Myz = ∫∫∫E x *p(x, y, z)dV
Mxz = ∫∫∫E y *p(x, y, z)dV
Mxy = ∫∫∫E z *p(x, y, z)dV
Center of Mass:
(X, Y, Z) =( Myz/m, Mxz/m, Mxy/m)
How to Change from Rectangular Coordinates to Cylindrical Coordinates in a triple Integral?
∫∫∫E f(x, y, z)dV = f (rcosθ, rsinθ, z) r dz dr dθ
E = {(r, θ, z) | a <= θ <= b, h1(θ) <= r <= h2(θ), u1( r cos(θ), r sin(θ) ) <= z <= u2( r cos(θ), r sin(θ) )